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We implement a new method by which to study the faint end of the field star luminosity function. The method relies on deep, multicolor photometry of fields projected against highly obscured, nearby mo...
We present OGLE-III Photometric Maps of the Galactic bulge fields observed during the third phase of the OGLE project. This paper describes the last, concluding set of maps based on OGLE-III data. Th...
We have analyzed data on 16,838 RR Lyrae variables observed toward the Galactic bulge during the third phase of the Optical Gravitational Lensing Experiment (OGLE) in 2001-2009. Using this type of sta...
Microlensing is now a very popular observational astronomical technique. The investigations accessible through this effect range from the dark matter problem to the search for extra-solar planets. In ...
Quasar Optical Variability and Black Hole Mass。
Surveys for Pulsed Optical Emission from Radio Pulsars。
The optical counterpart of sax j1808.4{3658 in quiescence:evidence of an active radio pulsar?
Cosmology with the GTC:A combined mm-optical galaxy cluster survey。
3C120:relation between optical variability and superluminal motions。
Infrared imaging and optical imaging and spectroscopy of (mostly) type I Planetary Nebulae. I. 。
Collisional Planetary Rings:The Role of the Width and the Optical Depth。

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